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首页> 外文期刊>AIP Advances >Obliquely propagating nonlinear ion-acoustic solitary and cnoidal waves in nonrelativistic magnetized pair-ion plasma with superthermal electrons
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Obliquely propagating nonlinear ion-acoustic solitary and cnoidal waves in nonrelativistic magnetized pair-ion plasma with superthermal electrons

机译:非相对论磁化成对离子等离子体中具有过热电子的非线性离子声孤立和斜向波的非线性传播

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The nonlinear propagation of ion-acoustic waves is considered in a magnetized system of collisionless and dissipative pair-ion plasma, composed of cold positively and negatively charged nonrelativistic ions, with superthermal electrons. obliquely propagating ion-acoustic solitary and cnoidal waves are investigated via a mechanical-motion analog Korteweg de Vries (KdV) approach. The characteristics of the emerged nonlinear magnetized waves are significantly modified by the effects of plasma parameters like the obliquity angle, superthermality parameter, negative to positive ions density ratio, electron density and it is also affected by the electron temperature. The obtained results can be generalized to be used to investigate the plasma waves nature in neutron stars, Saturn’s and Pulsars magnetospheres in addition to the laboratory plasmas.
机译:在无碰撞和耗散的成对离子等离子体的磁化系统中考虑了离子声波的非线性传播,该等离子体由冷的带正电和带负电的非相对论性离子以及过热电子组成。通过机械运动模拟Korteweg de Vries(KdV)方法研究了斜传播的离子声孤立波和星状波。出现的非线性磁化波的特性受到诸如倾斜角,超热参数,负离子对正离子的密度比,电子密度等等离子体参数的影响而显着改变,并且还受到电子温度的影响。除实验室等离子体外,所得结果还可推广用于研究中子星,土星和脉冲星磁层中的等离子体波性质。

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